Open Access

Table 3

Forecast on the future precision of optical GRB cosmology.

Sample OPT OPTtrim10 OPTtrim25
Reaching precision of Conley (before launch of THESEUS)

Original estimates (n=1) 271 330 244

n=1 + LCR + ML 99 158 72
Years to reach (n=1 + LCR + ML) 2032 2037 2030

Original estimates (n=2) 142 112 36

n=2 + LCR* 30 79 3
Years to reach (n=2 + LCR) 2028 2024 2005

Reaching precision of Betoule (after launch of THESEUS)

Original estimates (n=1) 1031 829 685

n=1 + LCR + ML 770 568 424
Years to reach (n=1 + LCR + ML) 2044 2041 2039

Original estimates (n=2) 284 393 350

n=2 + LCR 118 227 184
Years to reach (n=2 + LCR) 2035 2037 2036

n=2 + LCR + ML 23 132 89
Years to reach (n=2 + LCR + ML) 2032 2034 2033

Reaching Scolnic precision (after launch of THESEUS)

Original estimates (n=2) 1086 1513 822

n=2 + LCR + ML 825 1252 561
Years to reach (n=2 + LCR + ML) 2045 2052 2041

Notes. Number of optical GRBs with a plateau and redshift needed to reach the precision of ΩM as obtained in studies by Conley et al. (2011); Betoule et al. (2014); Scolnic et al. (2018) (for SNe Ia). This is an extension of the table provided in Dainotti et al. (2022a). The term n=1 indicates that the error bars on the GRB plateau parameters are full width, while n=2 indicates that the error bars are halved. The “LCR” indicates that the estimates for the number of GRBs have been boosted by using LCR, while “ML” indicates that the estimates have been boosted by using ML.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.